{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:R6TVPWWJMDN4HB3JEEQNAMUVBG","short_pith_number":"pith:R6TVPWWJ","schema_version":"1.0","canonical_sha256":"8fa757dac960dbc387692120d0329509934a45bedb0c038c36df3eba84014b4d","source":{"kind":"arxiv","id":"1409.0383","version":4},"attestation_state":"computed","paper":{"title":"What frequencies of standing surface waves can the subsolar magnetopause support?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.geo-ph","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Ferdinand Plaschke, Martin Archer","submitted_at":"2014-09-01T12:28:32Z","abstract_excerpt":"It is has been proposed that the subsolar magnetopause may support its own eigenmode, consisting of propagating surface waves which reflect at the northern/southern ionospheres forming a standing wave. While the eigenfrequencies of these so-called Kruskal-Schwartzschild (KS) modes have been estimated under typical conditions, the potential distribution of frequencies over the full range of solar wind conditions is not know. Using models of the magnetosphere and magnetosheath applied to an entire solar cycle's worth of solar wind data, we perform time-of-flight calculations yielding a database "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1409.0383","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2014-09-01T12:28:32Z","cross_cats_sorted":["physics.geo-ph","physics.plasm-ph"],"title_canon_sha256":"92d747b35bf2730b0f15ceaae889822c46c586a73dd2bef1895865bd047b7f2c","abstract_canon_sha256":"9a58e2fcc4807055ec78d1a6f0bae495acd6e0f65a65134f275ae46bdeb68a38"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:18:04.153698Z","signature_b64":"tqENxu7jzYh6WtFrqn+XZjbsevWha+voaiwBH1eYah7+QmTCWuNfnqQ2RpaZ+CxjFedPJ/VV1GSJZBNih/eLAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8fa757dac960dbc387692120d0329509934a45bedb0c038c36df3eba84014b4d","last_reissued_at":"2026-05-18T02:18:04.152965Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:18:04.152965Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"What frequencies of standing surface waves can the subsolar magnetopause support?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.geo-ph","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Ferdinand Plaschke, Martin Archer","submitted_at":"2014-09-01T12:28:32Z","abstract_excerpt":"It is has been proposed that the subsolar magnetopause may support its own eigenmode, consisting of propagating surface waves which reflect at the northern/southern ionospheres forming a standing wave. While the eigenfrequencies of these so-called Kruskal-Schwartzschild (KS) modes have been estimated under typical conditions, the potential distribution of frequencies over the full range of solar wind conditions is not know. Using models of the magnetosphere and magnetosheath applied to an entire solar cycle's worth of solar wind data, we perform time-of-flight calculations yielding a database "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.0383","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1409.0383","created_at":"2026-05-18T02:18:04.153067+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.0383v4","created_at":"2026-05-18T02:18:04.153067+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.0383","created_at":"2026-05-18T02:18:04.153067+00:00"},{"alias_kind":"pith_short_12","alias_value":"R6TVPWWJMDN4","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"R6TVPWWJMDN4HB3J","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"R6TVPWWJ","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG","json":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG.json","graph_json":"https://pith.science/api/pith-number/R6TVPWWJMDN4HB3JEEQNAMUVBG/graph.json","events_json":"https://pith.science/api/pith-number/R6TVPWWJMDN4HB3JEEQNAMUVBG/events.json","paper":"https://pith.science/paper/R6TVPWWJ"},"agent_actions":{"view_html":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG","download_json":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG.json","view_paper":"https://pith.science/paper/R6TVPWWJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.0383&json=true","fetch_graph":"https://pith.science/api/pith-number/R6TVPWWJMDN4HB3JEEQNAMUVBG/graph.json","fetch_events":"https://pith.science/api/pith-number/R6TVPWWJMDN4HB3JEEQNAMUVBG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG/action/storage_attestation","attest_author":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG/action/author_attestation","sign_citation":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG/action/citation_signature","submit_replication":"https://pith.science/pith/R6TVPWWJMDN4HB3JEEQNAMUVBG/action/replication_record"}},"created_at":"2026-05-18T02:18:04.153067+00:00","updated_at":"2026-05-18T02:18:04.153067+00:00"}